What Does Radiation Do to Cells?

Radiation is energy traveling as waves or particles that interacts with the biological machinery of living cells. This interaction deposits energy, disrupting the cell’s normal state. This energy causes damage ranging from temporary molecular disruptions to permanent changes in the cell’s genetic code. The fate of an exposed cell is determined by the balance between the initial damage and the cell’s capacity to recognize and repair the injury.

The Direct and Indirect Mechanisms of Cellular Damage

Radiation transfers its energy to a cell through two distinct processes: direct action and indirect action. Direct action occurs when the radiation particle physically strikes and ionizes a molecule important for the cell’s survival, directly breaking chemical bonds. Direct effects are more common with high-Linear Energy Transfer (LET) radiation, such as alpha particles, which deposit energy densely over a short path.

The most common mechanism of cellular damage, particularly with low-LET radiation like X-rays and gamma rays, is indirect action. This process begins when radiation interacts with the cell’s most abundant molecule, water, causing radiolysis. Radiolysis splits the water molecule into highly reactive fragments known as free radicals. Hydroxyl radicals (\(\cdot\)OH) are the most damaging of these free radicals, quickly moving to attack sensitive cellular components nearby. Indirect action, mediated primarily by hydroxyl radicals, accounts for approximately two-thirds of the total biological damage to DNA.

Primary Molecular Targets and Immediate Harm

The primary target within the cell for radiation-induced damage is the deoxyribonucleic acid (DNA) molecule. Damage to the DNA is the primary event leading to cell death or mutation because of its central role in storing and transmitting genetic information. The large size of the DNA molecule and its location within the nucleus make it a significant target for both direct ionization and free radical attack.

Radiation exposure causes various lesions, the most severe being strand breaks. A single-strand break (SSB) occurs when the sugar-phosphate backbone is severed on one side of the double helix. While SSBs are generally easy to repair, the double-strand break (DSB) is far more dangerous, involving a break in both strands that effectively cuts the chromosome in two. DSBs are the most lethal form of damage because they are difficult to repair accurately and can lead to the loss or rearrangement of large sections of the genome.

Beyond the DNA, radiation can damage cell membranes through lipid peroxidation, compromising structural integrity and permeability. Proteins and enzymes can also be denatured by free radicals, leading to a loss of function that impairs the cell’s ability to maintain homeostasis.

Cellular Response: Repair, Senescence, and Programmed Death

Following the detection of DNA damage, the cell initiates the DNA Damage Response (DDR). This response involves activating cell cycle checkpoints, which pause the cell’s progression through division to allow time for repair. Checkpoints in the G1, S, and G2 phases prevent a damaged cell from replicating or dividing, stopping faulty genetic material from being passed on.

The cell employs specialized pathways to fix double-strand breaks. One major mechanism is Non-Homologous End Joining (NHEJ), a quick but often error-prone process that simply ligates the two broken ends back together. NHEJ is active throughout the cell cycle and is the predominant DSB repair pathway in most mammalian cells.

The second major pathway, Homologous Recombination (HR), is a more accurate method but occurs only during the S and G2 phases when a sister chromatid is available as a template. HR uses the undamaged DNA sequence as a guide to precisely repair the break, reducing the chance of mutation. The cell’s decision to use NHEJ or HR is dictated by the cell cycle phase and the complexity of the damage.

If the damage is too extensive or cannot be repaired accurately, the cell prevents its survival through two mechanisms. One outcome is apoptosis, or programmed cell death, a controlled self-destruction process that eliminates the cell without causing inflammation. Alternatively, the cell may enter cellular senescence, an irreversible growth arrest where cells remain metabolically active but can no longer divide.

Long-Term Biological Outcomes

When the cell’s repair mechanisms fail or introduce errors, the surviving cell carries a permanent alteration in its genetic code, known as a mutation. A misrepaired double-strand break can result in chromosomal aberrations, such as deletions or translocations, which are stable changes passed on to all daughter cells. These accumulated mutations can affect genes that control cell growth, division, and death.

Genomic instability is the tendency of the cell’s descendants to acquire new mutations at an accelerated rate. This instability can manifest many generations after the initial radiation exposure, even in cells that did not receive a direct hit (the bystander effect). The accumulation of mutations and genomic instability are the foundations for radiation carcinogenesis, the process that can lead to cancer development.

If a mutation occurs in a key gene regulating cell division or suppressing tumors, the cell may gain a growth advantage. The combination of a heritable mutation and a persistently unstable genome can initiate the multi-step process of cancer, which may take years or decades to fully manifest.